Theia 586

0.13 UTI

0.3

C_N

0.05

C_dens

0.25

C_C3

0.03

C_lit

1.0

C_dup

N_m (P>50%) 30

Core radius and density 3.8 [pc], 0.3 [pc^-2]

C3 classification CC

C_N 0.3 Poorly populated
C_dens 0.05 Very loose
C_C3 0.25 Low quality
C_lit 0.03 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Theia 586 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Close Moderate extinction Near-solar metallicity Intermediate age

Palma et al. (2025)
Classified as optical pair (not dynamically associated) P91, along with CWNU_1252.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Data

🔍 Search references for Theia 586 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	39.854	62.577	1.203	-2.563	0.812	-23.064
Cavallo et al.	2024	39.809	62.705	1.207	–	–	–
Hunt & Reffert	2023	39.314	62.496	1.207	-2.571	0.831	-21.16
Kounkel & Covey	2019	39.874	62.761	1.217	–	–	-35.564

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	B_frac	BSS
UCC	99999–	0.82	1.39	0.79	229	0.050	–	–	–
Cavallo et al.	2024	0.87	1.39	–	229	0.050	–	–	–
Hunt & Reffert	2023	0.80	1.45	0.79	112	–	–	–	–
Kounkel & Covey	2019	0.82	1.07	–	248	–	–	–	–

Visualization

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